10.3 SPACE CURVES
so we finally obtain
dˆb
ds
=−τˆn. (10.14)
Taking the dot product of each side withnˆ, we see that the torsion of a curve is
given by
τ=−nˆ·
dˆb
ds
.
We may also define the quantityσ=1/τ, which is called theradius of torsion.
Finally, we consider the derivativednˆ/ds.Sincenˆ=ˆb׈twe have
dnˆ
ds
=
dbˆ
ds
׈t+ bˆ×
dˆt
ds
=−τnˆ×ˆt+ bˆ×κˆn
=τˆb−κˆt. (10.15)
In summary,ˆt,nˆandbˆand their derivatives with respect tosare related to one
another by the relations (10.13), (10.14) and (10.15), theFrenet–Serret formulae,
dˆt
ds
=κˆn,
dnˆ
ds
=τˆb−κˆt,
dbˆ
ds
=−τnˆ. (10.16)
Show that the acceleration of a particle travelling along a trajectoryr(t)is given by
a(t)=
dv
dt
ˆt+v
2
ρ
nˆ,
wherevis the speed of the particle,ˆtis the unit tangent to the trajectory,nˆis its principal
normal andρis its radius of curvature.
The velocity of the particle is given by
v(t)=
dr
dt
=
dr
ds
ds
dt
=
ds
dt
ˆt,
whereds/dtis the speed of the particle, which we denote byv,andˆtis the unit vector
tangent to the trajectory. Writing the velocity asv=vˆt, and differentiating once more
with respect to timet,weobtain
a(t)=
dv
dt
=
dv
dt
ˆt+vd
ˆt
dt
;
but we note that
dˆt
dt
=
ds
dt
dˆt
ds
=vκnˆ=
v
ρ
nˆ.
Therefore, we have
a(t)=
dv
dt
ˆt+v
2
ρ
nˆ.
This shows that in addition to an accelerationdv/dtalong the tangent to the particle’s
trajectory, there is also an accelerationv^2 /ρin the direction of the principal normal. The
latter is often called thecentripetalacceleration.